Study 000374:

ACRONYM:  cam_sigmoid_study_v1 

Using EIS data has shown the existence of sigmoidal structures at
lower coronal temperatures and interpreted as cooling plasma on newly
reconnected field lines within a flux rope. However, more specific
observations simultaneously at different temperatures are needed to
comprehend this result.

TARGET: 		Active Region
EXPOSURE TIME: 		10s
RASTER: 		Scanning
SLIT: 			2"
FOV: 			400"x400"
RASTER DURATION: 	41m 33s 
Data Volume:		125 Mbits
Data rate:		50 Kbits/s

Line list:
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FeX,184.54; FeXII,186.88; FeXI,188.23; FeXII,195.12; FeIX,196.81;
FeXIII,202.04; FeXIII,203.83; FeXVII,254.87; FeXVI,262.98; FeXXIII,263.76;
FeXIV,274.20; SiVII,275.35; FeXV,284.16

Pointing:
---------

Small to medium size active regions. The pointing should be such that
the active region is located in the middle of the raster, Preferably at
the centre.

Instructions to planner:
------------------------

Adjust the raster repeat to fill the available time slot. However,
it would be very helpful scientifically if at least **4** repeats 
can be supported

WARNING:
--------

Total data volume for the desired 4 repeats is ~500 Mbits